Hyperbolic L-space knots and their Upsilon invariants
Abstract.
For a knot in the –sphere, the Upsilon invariant is a piecewise linear function defined on the interval . For an L–space knot, the Upsilon invariant is determined only by the Alexander polynomial of the knot. We exhibit infinitely many pairs of hyperbolic L–space knots such that two knots of each pair have distinct Alexander polynomials, so they are not concordant, but share the same Upsilon invariant. Conversely, we examine the restorability of the Alexander polynomial of an L–space knot from the Upsilon invariant through the Legendre–Fenchel transformation.
2020 Mathematics Subject Classification:
Primary 57K10; Secondary 57K181. Introduction
For a knot in the –sphere , Ozsváth, Stipsicz and Szabó [30] defined the Upsilon invariant , which is a piecewise linear real-valued function defined on the interval . This invariant is additive under connected sum of knots, and the sign changes for the mirror image of a knot. Also, it gives a lower bound for the genus, the concordance genus and the four genus. Although it is originally defined through some modified knot Floer complex, Livingston [23] later gives an alternative interpretation on the full knot Floer complex .
As the most important feature, the Upsilon invariant is a concordance invariant, so it is obviously not strong to distinguish knots, although it has been used to establish various powerful results about independent elements in the knot concordance group [11, 16, 30, 38]. For a smoothly slice knot, the Upsilon invariant is the zero function. It depends only on the signature for an alternating knot or a quasi-alternating knot [30]. Also, it is determined by the –invariant for concordance genus one knots [11].
In this paper, we concentrate on L–space knots, which are recognized to form an important class of knots in recent research. A knot is called an L–space knot if it admits a positive surgery yielding an L–space. Positive torus knots are typical examples of L–space knots. Note that any non-trivial L–space knot is prime [19] and non-slice [27]. For an L–space knot, the Upsilon invariant is determined only by the Alexander polynomial [30, Theorem 6.2].
There is another interesting route to lead to the Upsilon invariant of an L–space knot. The Alexander polynomial gives the formal semigroup [37], in turn, the gap function [7]. These notions have the same information as the Alexander polynomial. Then the Upsilon invariant is obtained as the Legendre–Fenchel transform of the gap function [6].
In general, the gap function for an L–space knot is not convex, so the further Legendre–Fenchel transformation on the Upsilon invariant does not return the original gap function. Thus there is a possibility that distinct gap functions, equivalently Alexander polynomials, correspond to the same Upsilon invariant. In other words, it is expected to exist non-concordant L–space knots with the same Upsilon invariant. We remark that the Alexander polynomial is a concordance invariant for L–space knots [19]. Our main result shows that this is possible among hyperbolic L–space knots.
Theorem 1.1.
There exist infinitely many pairs of hyperbolic L–space knots and such that they have distinct Alexander polynomials but share the same non-zero Upsilon invariant.
Thus two hyperbolic L–space knots in our pair are not concordant. In the literature, there are plenty of examples of non-concordant knots sharing the same Upsilon invariant [1, 11, 17, 38, 39, 40, 42]. However, they use either connected sums of torus knots or satellite knots, which are not hyperbolic.
Since the Upsilon invariant is determined only by the Alexander polynomial for an L–space knot, any pair of L–space knots sharing the same Alexander polynomial have the same Upsilon invariant. For example, the hyperbolic L–space knot t09847 in the SnapPy census has the same Alexander polynomial as the –cable of , which is an L–space knot. There are infinitely many such pairs consisting of a hyperbolic L–space knot and an iterated torus L–space knot (found in [3]).
However, we checked Dunfield’s list of hyperbolic L–space knots ([2, 3]), and confirmed that there is no duplication among their Alexander polynomials and that there is no one sharing the same Alexander polynomial as a torus knot. This leads us to pose a question.
Question 1.2.
-
(1)
Do there exist hyperbolic L–space knots which have the same Alexander polynomial, equivalently, which are concordant?
-
(2)
Does there exist a hyperbolic L–space knot which is concordant to a torus knot?
In general, it is rare that the Alexander polynomial of an L–space knot is restorable from the Upsilon invariant. The reason is the fact that the gap function, which has the same information as the Alexander polynomial, is not convex, and the Upsilon invariant depends only on the convex hull of the gap function. In fact, our knots in Theorem 1.1 are designed so that they have distinct Alexander polynomials, but their gap functions share the same convex hull, so the same Upsilon invariant.
On the other hand, there is a chance that the gap function is restorable from its convex hull. This means that the Alexander polynomial is also restorable from the Upsilon invariant through the Legendre–Fenchel transformation. We can give infinitely many such gap functions, equivalently Alexander polynomials, but there lies a hard question, called a geography question, whether such gap function can be realized by an L-space knot or not.
In this paper, we can give only two hyperbolic L–space knots whose Alexander polynomials are restorable from the Upsilon invariants.
Theorem 1.3.
Let be the hyperbolic L–space knot t09847 or v2871 in the SnapPy census. Then the Alexander polynomial of is restorable from the Upsilon invariant . That is, the equation implies (up to units) for any other L–space knot .
In Section 2, we give a pair of knots and , which yields an infinite family of pairs of L–space knots. In Section 3, we calculate their Alexander polynomials and the formal semigroups, which are sufficient to prove that the knots are hyperbolic. Section 4 gives the gap functions and their convex hulls, and confirm that they correspond to the same Upsilon invariant. Section 5 shows that the knots admit L–space surgery through the Montesinos trick, which completes the proof of Theorem 1.1. In the last section, we investigate the restorability of Alexander polynomial from the Upsilon invariant, and prove Theorem 1.3.
2. The pairs of hyperbolic L-space knots
For any integer integer , the surgery diagrams illustrated in Figure 1 define our knots and , where the surgery coefficient on is and that on is . The images of after these surgeries in (1) and (2) of Figure 1 give and , respectively. (The link with orientations is placed in a strongly invertible position, and the axis is depicted there for later use.)

Hence, our knots are the closures of –braids
where is the standard generator of the –strand braid group. When , is m240, and is t10496 in the SnapPy census [9].
Theorem 1.1 immediately follows from the next.
Theorem 2.1.
For each integer , the knots and defined above satisfy the following.
-
(1)
They are hyperbolic.
-
(2)
–surgery on and –surgery on yield L–spaces.
-
(3)
Their Alexander polynomials are distinct.
-
(4)
They share the same Upsilon invariant.
Proof.
Each diagram in Figure 1 has a single negative crossing, but it can be cancelled obviously with some positive crossing. Hence both knots are represented as the closures of positive braids, which implies that they are fibered [33]. Then it is straightforward to calculate their genera , and we see that .
3. Alexander polynomials
We calculate the Alexander polynomials of and . Since and are obtained from by performing some surgeries on and , we mimic the technique of [3].
Theorem 3.1.
The Alexander polynomial of is given as
Proof.
Let be the oriented link illustrated in Figure 1(1). Its multivariable Alexander polynomial is
where the variables correspond to the (oriented) meridians of , , , respectively. (We used [9, 18] for the calculation.)
Performing –surgery on and –surgery on changes the link to . These two links have homeomorphic exteriors. Hence the induced isomorphism of the homeomorphism on their homology groups relates the Alexander polynomials of two links [12, 25].
Let , and be the homology classes of meridians of , , , respectively. We assume that each meridian has linking number one with the corresponding component. Furthermore, let , and be the homology classes of their oriented longitudes. We see that and .
Let , and be the homology classes of meridians of , and . Then we have that , , . Hence
Thus we have the relation between the Alexander polynomials as
(3.1) |
Since and , the Torres condition [36] gives
We put
Then a direct calculation shows
Thus
We have the conclusion as desired. ∎
Theorem 3.2.
The Alexander polynomial of is given as
Proof.
The argument is very similar to the proof of Theorem 3.1, so we omit the details.
Let be the oriented link illustrated in Figure 1(2). Its multivariable Alexander polynomial is
where correspond to the meridians of , respectively.
Then
Again, we put
A direct calculation shows
This shows that
Thus as desired. ∎
We recall the notion of formal semigroup for an L–space knot [37]. Let be an L–space knot in the –sphere. Then the Alexander polynomial of has a form of
(3.2) |
where , and is the genus of [27]. We expand the Alexander function into a formal power series as
(3.3) |
(This is called the Milnor torsion in [10].) The set is a subset of non-negative integers, called the formal semigroup of . For example, for a torus knot , its formal semigroup is known to be the actual semigroup of rank two,
(see [7, 37]). If an L–space knot is an iterated torus knot, then its formal semigroup is also a semigroup [37], but in general, the formal semigroup of a hyperbolic L–space knot is hardly a semigroup [3, 35].
Let and .
Proposition 3.3.
The formal semigroup of is given as
Proof.
We use in the proof of Theorem 3.1. For
we expand each term as follows;
The conclusion immediately follows from these. ∎
Proposition 3.4.
The formal semigroup of is given as
Proof.
Corollary 3.5.
For , the formal semigroup of is not a semigroup.
Proof.
Lemma 3.6.
Both of and are hyperbolic.
Proof.
By Corollary 3.5, the formal semigroup of is not a semigroup. Hence is not a torus knot, because the formal semigroup of a torus knot is a semigroup.
Assume for a contradiction that is a satellite knot. Since is the closure of a –braid, its bridge number is at most four. By [32], it is equal to four. Moreover, the companion is a –bridge knot and the pattern knot has wrapping number two. We know that both of the companion and the pattern knot are L–space knots and the pattern is braided by [5, 16]. Thus the companion is a –bridge torus knot [27], and is its –cable. By [37], the formal semigroup of an iterated torus L–space knot is a semigroup, which contradicts Corollary 3.5. We have thus shown that is hyperbolic. ∎
4. Upsilon invariants
In this section, we verify that the Upsilon invariants of and are the same. We will not calculate the Upsilon invariants. Instead, we determine the gap functions defined later. For an L–space knot, the Upsilon invariant is the Legendre–Fenchel transform of the gap function [6]. Hence if the gap functions of and share the same convex hull, then their Upsilon invariants also coincide.
First, we quickly review the Legendre–Fenchel transformation.
For a function , the Legendre–Fenchel transform is defined as
The domain of is the set .
The Legendre transform is defined only for differentiable convex functions, but the Legendre–Fenchel transform can be defined even for non-convex functions with non-differentiable points. The transform is always a convex function. Hence, if is not convex, then the double Legendre–Fenchel transform does not return . In this case, gives the convex hull of the function . Thus we see that depends only on the convex hull of .
Next, we recall the notion of gap function introduced in [7].
Let be an L–space knot with formal semigroup . Then is called the gap set. In fact, , where , and . The part is called the gap sequence. Then it is easy to restore the Alexander polynomial as
From the gap set , we define the function by
and let . Then we extend linearly to obtain a piecewise linear function on . That is, for , if , then on , and if , then for . Borodzik and Hedden [6] showed that the Upsilon invariant of is the Legendre–Fenchel transform of the function . We call this function the gap function of .
Example 4.1.
Let be the –pretzel knot. It admits a lens space surgery, so is an L–space knot. Also, it has genus . The Alexander polynomial is . Then , and . Tables 1 and 2 show the values of and the gap function .
9 | 8 | 7 | 6 | 5 | 4 | 3 | 2 | 1 | 0 | |||||
0 | 1 | 1 | 1 | 2 | 2 | 3 | 3 | 4 | 5 | 5 | 6 | 7 |
0 | 1 | 2 | 3 | 4 | 5 | 6 | 7 | |||||||
0 | 2 | 2 | 2 | 4 | 4 | 6 | 6 | 8 | 10 | 10 | 12 | 14 |
Figure 2 shows the graph of the gap function and its convex hull (broken line). Here, the convex hull of the gap function is given by

Then the Legendre–Fenchel transformation gives the Upsilon invariant
In general, the gap function of an L–space knot has a specific property.
-
•
The slope of each segment of the graph is or .
Although this observation is easy to see, we will use it essentially in Section 6 with further investigation.
Now, we calculate the gap functions of and .
From Proposition 3.3, the gap set is
Hence the values of is given as in Table 3. When is an integer not in the table, takes the same value as the nearest with . For example, for .
0 | 1 | 2 |
---|
3 | 2 | 1 | |||||||
Let with . Then the gap function takes the values as in Table 4.
0 | 2 | 4 |
---|
Figure 3 shows the graph of the gap function of when .

0 | 1 | 2 |
3 | 2 | 1 | |||||||
0 | 2 | 4 |

Lemma 4.2.
For , the convex hull of the gap function for is given by
Proof.
Consider the gap function of . Let be the convex hull. From Table 4, it is obvious that for and for .
On the interval , the gap function has the branch as shown in Figure 4(b). It repeats on the intervals . Thus on .
On and , the branch is of Figure 4(c). Hence on .
Similarly, the branch of Figure 4(d) repeats on the intervals . This gives on .
On and , the branch of Figure 4(f) appears. Thus on .
Finally, the branch of Figure 4(g) repeats on . Then on . We have thus shown that the convex hull is given as claimed for .
Next, consider the gap function of . For , the situation is the same as .
On , the branch of Figure 4(e) appears. This branch repeats on . However, the convex hull is the same as .
For the remaining range , the gap function is the same as one of . In conclusion, the gap functions of and are distinct only on , but their convex hulls coincide there. ∎
Corollary 4.3.
The Upsilon invariants of and coincide.
Proof.
The Upsilon invariant is the Legendre–Fenchel transform of the gap function . In fact, it depends only on the convex hull of the gap function. By Lemma 4.2, and have the same convex hull for their gap functions. Thus the conclusion follows. ∎
5. The Montesinos trick
In this section, we verify that and admit positive Dehn surgeries yielding L–spaces by using the Montesinos trick [24]. For a surgery diagram on a strongly invertible link, the Montesinos trick describes the resulting closed –manifold as the double branched cover of another knot or link obtained from tangle replacements corresponding to the surgery coefficients on some link obtained from the quotient of the original strongly invertible link under the strong involution (see also [26, 41]).
In Figure 1(1) and (2), each link is placed in a strongly invertible position, where the dotted line indicates the axis of the involution.
Lemma 5.1.
For , –surgery yields an L–space.
Proof.
Assign the surgery coefficient on in Figure 1(1). After performing –surgery on and –surgery on , our knot has surgery coefficient .
The left of Figure 5 shows the knot obtained from the tangle replacements. In the diagram of Figure 1, we should remark that the component has writhe . Hence the tangle replacement corresponding to the quotient of is realized by the –tangle (depicted as the dotted circle).
Then Figures 5, 6, and 7 show the deformation of the knot. Finally, we obtain the Montesinos knot . Thus the double branched cover is the Seifert fibered manifold . We use the notation of [22]. That is, is obtained by –surgery on the unknot with three meridians having –surgery on the -th one. Then . By the criterion of [21, 22], is an L–space. ∎



Lemma 5.2.
For , –surgery yields an L–space.
Proof.
Assign the surgery coefficient on in Figure 1(2). After performing –surgery on and –surgery on , has surgery coefficient .
The process is similar to that for . We should remark that the tangle replacement to the quotient of is realized by –tangle as depicted in the dotted circle in Figure 8 (left), because has writhe in the diagram.

Let be the link as illustrated in the right of Figure 8. We need to verify that the double branched cover of is an L–space.
For the crossing of encircled in Figure 8 (right), we perform two resolutions as shown in Figure 9. Let and be the resulting knots. It is straightforward to calculate , and from the checkerboard colorings on the diagrams of Figures 8, 11 and 12. Thus the equation holds. This implies that if the double branched covers of and are L–spaces, then so is the double branched cover of ([8, 27, 28]).

Claim 5.3.
The knot is the –pretzel knot. Its double branched cover is an L–space.
Proof.
If , then is the connected sum of torus knots and . Then the double branched cover is the connected sum of lens spaces , which is an L–space. If , then is the –bridge knot , so the double cover is a lens space. Hence we assume .
Since is the Montesinos knot , its double branched cover is the Seifert fibered manifold . Then .
We use the criterion of [22]. If , then set , and . Then . If there are no coprime integers such that , and , then is an L–space. However, the first two give , so there are no such integers.
Finally, assume . Set , and . Then . If , then . For and , does not hold. Thus there are no coprime integers as desired, which implies that is an L–space. ∎


Claim 5.4.
The double branched cover of is an L–space.
Proof.
For the crossing encircled in Figure 12, we further perform the resolutions, which yield and . Clearly, . Hence .

We can confirm that is the connected sum of the Hopf link and a Montesinos knot as shown in Figures 13 and 14. From the diagram of Figure 14, we see that . Recall that . Hence the equation holds.


From Claim 5.3, the double branched cover of is an L–space. It remains to show that the double branched cover of is an L–space.
The double branched cover of the Montesinos knot is the Seifert fibered manifold . Since is homeomorphic to , set , and . Then . We apply the criterion of [22] again. If , then . Hence there are no coprime integers such that . Thus is an L–space.
The double branched cover of is the connected sum of a lens space and . Since the sum of L–spaces is an L–space [27], we have the conclusion. ∎
6. Restorability of Alexander polynomials
In this section, we investigate the restorability of Alexander polynomial of an L–space knot from the Upsilon invariant.
As easy examples, we examine two torus knots.
Example 6.1.
(1) Let . Then , so and . It is easy to calculate as
The Legendre–Fenchel transformation on gives a function
Of course, this is the convex hull of the gap function of . Figure 15 shows the graphs of gap function of and .

We consider the possibility of another gap function whose convex hull is . First, it forces , and . Recall that each segment of the graph of a gap function has slope or as mentioned in Section 4. Hence . Since a gap function is increasing, . Similarly, it is necessary that and . Thus coincides with the gap function of .
This means that if another L–space knot has the same Upsilon invariant as , then , because a gap function uniquely determines the Alexander polynomial.
(2) Let . We have , so , and . Then is given as
Figure 15 shows the graphs of gap function of and the convex hull, which is the Legendre–Fenchel transform of . As in (1), the convex hull uniquely restores the gap function.
In general, it is rare that the convex hull uniquely restores a gap function. In Example 4.1, we determined the gap function and its convex hull of the –pretzel knot (see Figure 2). It is possible that another gap function takes the same values on integers except , keeping the same convex hull. This new gap function corresponds to the Alexander polynomial . This polynomial satisfies the condition of [20], but there is no hyperbolic L–space knot in Dunfield’s list whose Alexander polynomial is . It seems to be a hard question whether there exists a hyperbolic L–space knot with . Of course, there exists a hyperbolic knot whose Alexander polynomial is by [13, 34]. Also, is the Alexander polynomial of the –cable of , which is not an L–space knot [15].
If we put off the realizability of the Alexander polynomial or the gap function by a hyperbolic L–space knot, then we can easily design many Alexander polynomials which are restorable from convex hulls.
It is a classical result that any polynomial satisfying and is realized by a knot in the –sphere as its Alexander polynomial. (Here, shows the equality up to units in the Laurent polynomial ring .) Furthermore, we assume that has the form of (3.2). Formally, we define the formal semigroup by (3.3), and in turn, its gap set and the gap function.
Proposition 6.2.
Let be an integer, and let . Then its gap function, defined formally, is uniquely determined from the convex hull.
Again, the polynomial in Proposition 6.2 satisfies the condition of [20], but it is open whether is realized by a hyperbolic L–space knot or not. (When , is the Alexander polynomial of .)
Proof.
By (3.3), the formal semigroup is , so the gap set is . Set . Then we can calculate the gap function as in Table 7.
0 | 2 | 4 |
Let be the convex hull. Then it is given by
Since each segment of the graph of any gap function has slope or , there is no other gap function whose convex hull is . ∎
Finally, we prove Theorem 1.3. For reader’s convenience, we record the braid words for the knots t09847 and v2871. Both are the closures of –braids, whose words are almost the same:
Proof of Theorem 1.3.
Let be the hyperbolic knot t09847 in the SnapPy census. The Alexander polynomial is , so the formal semigroup is .
Figure 16 shows the graph of the gap function and its convex hull (we omit the details). It consists of branches of types (a), (b), (c), (f), (g) and (h) of Figure 4 from the left. Then there is no other gap function with the same convex hull.

Next, let be the hyperbolic knot v2871. The Alexander polynomial is , so the formal semigroup is and the gap set is . Figure 17 shows the graph of the gap function and its convex hull. In this case, the graph consists of branches of types (a), (b), (c), (e), (f), (g) and (h) of Figure 4 from the left. Again, there is no other gap function with the same convex hull. ∎

Acknowledgement
The author would like to thank Kouki Sato for valuable communication.
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